Vertaling en analyse van woorden door kunstmatige intelligentie ChatGPT
Op deze pagina kunt u een gedetailleerde analyse krijgen van een woord of zin, geproduceerd met behulp van de beste kunstmatige intelligentietechnologie tot nu toe:
- hoe het woord wordt gebruikt
- gebruiksfrequentie
- het wordt vaker gebruikt in mondelinge of schriftelijke toespraken
- opties voor woordvertaling
- Gebruiksvoorbeelden (meerdere zinnen met vertaling)
- etymologie
x ray mirror - vertaling naar arabisch
![Mock-up of ''XMM-Newton'' at the ''[[Cité de l'espace]]'', [[Toulouse]].](https://commons.wikimedia.org/wiki/Special:FilePath/XMM-Newton.jpg?width=200 "Mock-up of ''XMM-Newton'' at the ''[[Cité de l'espace]]'', [[Toulouse]].")
![Model of the arrangement of water molecules in ice, revealing the [[hydrogen bond]]s (1) that hold the solid together.](https://commons.wikimedia.org/wiki/Special:FilePath/3D model hydrogen bonds in water.svg?width=200 "Model of the arrangement of water molecules in ice, revealing the [[hydrogen bond]]s (1) that hold the solid together.")
![The incoming beam (coming from upper left) causes each scatterer to re-radiate a small portion of its intensity as a spherical wave. If scatterers are arranged symmetrically with a separation ''d'', these spherical waves will be in sync (add constructively) only in directions where their path-length difference 2''d'' sin θ equals an integer multiple of the [[wavelength]] λ. In that case, part of the incoming beam is deflected by an angle 2θ, producing a ''reflection'' spot in the [[diffraction pattern]].](https://commons.wikimedia.org/wiki/Special:FilePath/Bragg diffraction 2.svg?width=200 "The incoming beam (coming from upper left) causes each scatterer to re-radiate a small portion of its intensity as a spherical wave. If scatterers are arranged symmetrically with a separation ''d'', these spherical waves will be in sync (add constructively) only in directions where their path-length difference 2''d'' sin θ equals an integer multiple of the [[wavelength]] λ. In that case, part of the incoming beam is deflected by an angle 2θ, producing a ''reflection'' spot in the [[diffraction pattern]].")
![tetrahedrally]] and held together by single [[covalent bond]]s, making it strong in all directions. By contrast, graphite is composed of stacked sheets. Within the sheet, the bonding is covalent and has hexagonal symmetry, but there are no covalent bonds between the sheets, making graphite easy to cleave into flakes.](https://commons.wikimedia.org/wiki/Special:FilePath/Diamond and graphite2.jpg?width=200 "tetrahedrally]] and held together by single [[covalent bond]]s, making it strong in all directions. By contrast, graphite is composed of stacked sheets. Within the sheet, the bonding is covalent and has hexagonal symmetry, but there are no covalent bonds between the sheets, making graphite easy to cleave into flakes.")
![backbone]] from its N-terminus to its C-terminus.](https://commons.wikimedia.org/wiki/Special:FilePath/Myoglobin.png?width=200 "backbone]] from its N-terminus to its C-terminus.")
![Rocknest]]", October 17, 2012).<ref name="NASA-20121030" />](https://commons.wikimedia.org/wiki/Special:FilePath/PIA16217-MarsCuriosityRover-1stXRayView-20121017.jpg?width=200 "Rocknest]]\", October 17, 2012).<ref name=\"NASA-20121030\" />")
![A protein crystal seen under a [[microscope]]. Crystals used in X-ray crystallography may be smaller than a millimeter across.](https://commons.wikimedia.org/wiki/Special:FilePath/Protein crystal.jpg?width=200 "A protein crystal seen under a [[microscope]]. Crystals used in X-ray crystallography may be smaller than a millimeter across.")
Definitie
Wikipedia
XMM-Newton, also known as the High Throughput X-ray Spectroscopy Mission and the X-ray Multi-Mirror Mission, is an X-ray space observatory launched by the European Space Agency in December 1999 on an Ariane 5 rocket. It is the second cornerstone mission of ESA's Horizon 2000 programme. Named after physicist and astronomer Sir Isaac Newton, the spacecraft is tasked with investigating interstellar X-ray sources, performing narrow- and broad-range spectroscopy, and performing the first simultaneous imaging of objects in both X-ray and optical (visible and ultraviolet) wavelengths.
Initially funded for two years, with a ten-year design life, the spacecraft remains in good health and has received repeated mission extensions, most recently in March 2023 and is scheduled to operate until the end of 2026. ESA plans to succeed XMM-Newton with the Advanced Telescope for High Energy Astrophysics (ATHENA), the second large mission in the Cosmic Vision 2015–2025 plan, to be launched in 2035. XMM-Newton is similar to NASA's Chandra X-ray Observatory, also launched in 1999.
As of May 2018, close to 5,600 papers have been published about either XMM-Newton or the scientific results it has returned.
